Difference: GalOneNotes (1 vs. 12)

Revision 1202 Apr 2009 - Main.AngelaBragaglia

 
META TOPICPARENT name="Gal1"

Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

Would be useful to delete a subset of table in Topcat.

Changed:
<
<
Would be useful to have more than 4 tables to cross-match in TOPCAT
>
>
Would be useful to have more than 4 tables to cross-match in TOPCAT (AB)
 
Changed:
<
<
Would be useful to "remember" last scatter plot in TOPCAT, so we can use the same axes if we change from one table to a similar one
>
>
Would be useful to "remember" last scatter plot in TOPCAT, so we can use the same axes if we change from one table to a similar one (AB)
 
Changed:
<
<
In Virgo: it would be useful to have different colours for the background and written parts (black on gray is not very readable).
>
>
In Virgo: it would be useful to have different colours for the background and written parts (black on gray is not very readable) (AB)
 
Changed:
<
<
In Virgo: it would be useful to get a list of the pointings/exposures shown in Stellarium; it would help to choose them
>
>
In Virgo: it would be useful to get a list of the pointings/exposures shown in Stellarium; it would help to choose them (AB)
 
Changed:
<
<
In Virgo: it would be useful to see also PI and program ID when an exposure is selected; or even the possibility of selecting by PI/ID if known.
>
>
In Virgo: it would be useful to see also PI and program ID when an exposure is selected; or even the possibility of selecting by PI/ID if known (AB)
  -- AidaSchool - 31 Mar 2009

  • Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec:
    vospec.jpg
  • Comparison of an observed SED with a theoretical model (Use Case 2)

  • An SDSS RGB image of NGC2420. Overplotted are the hot star candidates.:
    im_all.jpg
  • An example for the collaboration betweenTopcat and Aladin
  • topcat_aladin.jpg
  • case1_hist_plx_Pleiades.jpg
  • case1_Xray_source.jpg

  • Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image.

IPHAS and 2MASS color-color diagrams for matched point sources (case 4) selected in a box 1 degree wide and centred at ra=38.78 and deg=61.43

    • Use case 5: The field of streams

META FILEATTACHMENT attachment="vospec.jpg" attr="" comment="Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec" date="1238599014" name="vospec.jpg" path="vospec.jpg" size="35840" stream="vospec.jpg" tmpFilename="/var/tmp/CGItemp8489" user="AngelaBragaglia" version="1"
META FILEATTACHMENT attachment="tuvikene_streams.png" attr="" comment="Use Case 5: The Field of Streams" date="1238600244" name="tuvikene_streams.png" path="tuvikene_streams.png" size="130281" stream="tuvikene_streams.png" tmpFilename="/var/tmp/CGItemp13144" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="IMF_case.jpg" attr="" comment="Comparison of an observed SED with a theoretical model (Use Case 2)" date="1238600342" name="IMF_case.jpg" path="IMF_case.jpg" size="119348" stream="IMF_case.jpg" tmpFilename="/var/tmp/CGItemp13617" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="ana.jpg" attr="" comment="Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image." date="1238600640" name="ana.jpg" path="ana.jpg" size="204032" stream="ana.jpg" tmpFilename="/var/tmp/CGItemp10897" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin.jpg" attr="" comment="usercase1_a" date="1238600827" name="Aladin.jpg" path="Aladin.jpg" size="50624" stream="Aladin.jpg" tmpFilename="/var/tmp/CGItemp19521" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="histogram.jpg" attr="" comment="usercase1_b" date="1238600859" name="histogram.jpg" path="histogram.jpg" size="23756" stream="histogram.jpg" tmpFilename="/var/tmp/CGItemp19669" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="color_color2.jpg" attr="" comment="usercase1_c" date="1238600881" name="color_color2.jpg" path="color_color2.jpg" size="49936" stream="color_color2.jpg" tmpFilename="/var/tmp/CGItemp19704" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin_after.jpg" attr="" comment="usercase1_d" date="1238600911" name="Aladin_after.jpg" path="Aladin_after.jpg" size="68656" stream="Aladin_after.jpg" tmpFilename="/var/tmp/CGItemp19721" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="VO_galaxy.png" attr="" comment="Galaxy and some foreground point sources." date="1238601001" name="VO_galaxy.png" path="VO_galaxy.png" size="683047" stream="VO_galaxy.png" tmpFilename="/var/tmp/CGItemp13959" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="im_all.jpg" attr="" comment="An SDSS RGB image of NGC2420. Overplotted are the hot star candidates." date="1238601083" name="im_all.jpg" path="im_all.jpg" size="19206" stream="im_all.jpg" tmpFilename="/var/tmp/CGItemp4593" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="topcat_aladin.jpg" attr="" comment="Collaboration between TOPCAT and Aladin" date="1238601577" name="topcat_aladin.jpg" path="topcat_aladin.jpg" size="395760" stream="topcat_aladin.jpg" tmpFilename="/var/tmp/CGItemp7499" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_Xray_source.jpg" attr="" comment="The Xray sources in the field correspond to rhe bright stars." date="1238602079" name="case1_Xray_source.jpg" path="case1_Xray_source.jpg" size="26188" stream="case1_Xray_source.jpg" tmpFilename="/var/tmp/CGItemp13621" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades" attr="h" comment="Histogram of the paralax. Blue are the bright stars." date="1238602249" name="case1_hist_plx_Pleiades" path="case1_hist_plx_Pleiades" size="23089" stream="case1_hist_plx_Pleiades" tmpFilename="/var/tmp/CGItemp13498" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Virgo2808.png" attr="" comment="Virgo : NGC2808 & search for dataset of high-res VLT spectra" date="1238602253" name="Virgo2808.png" path="Virgo2808.png" size="917789" stream="Virgo2808.png" tmpFilename="/var/tmp/CGItemp13232" user="AngelaBragaglia" version="1"
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades.jpg" attr="" comment="Histogram of the paralax. Blue are the bright stars." date="1238602468" name="case1_hist_plx_Pleiades.jpg" path="case1_hist_plx_Pleiades.jpg" size="23089" stream="case1_hist_plx_Pleiades.jpg" tmpFilename="/var/tmp/CGItemp13651" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Picture_5.png" attr="" comment="Halpha emitters in the IPHAS and 2MASS diagrams" date="1238658398" name="Picture_5.png" path="Picture 5.png" size="261604" stream="Picture 5.png" tmpFilename="/var/tmp/CGItemp9953" user="AidaSchool" version="1"

Revision 1102 Apr 2009 - Main.DeborahBaines

 
META TOPICPARENT name="Gal1"

Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

Would be useful to delete a subset of table in Topcat.

Would be useful to have more than 4 tables to cross-match in TOPCAT

Would be useful to "remember" last scatter plot in TOPCAT, so we can use the same axes if we change from one table to a similar one

In Virgo: it would be useful to have different colours for the background and written parts (black on gray is not very readable).

In Virgo: it would be useful to get a list of the pointings/exposures shown in Stellarium; it would help to choose them

In Virgo: it would be useful to see also PI and program ID when an exposure is selected; or even the possibility of selecting by PI/ID if known.

-- AidaSchool - 31 Mar 2009

  • Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec:
    vospec.jpg
  • Comparison of an observed SED with a theoretical model (Use Case 2)

  • An SDSS RGB image of NGC2420. Overplotted are the hot star candidates.:
    im_all.jpg
  • An example for the collaboration betweenTopcat and Aladin
  • topcat_aladin.jpg
  • case1_hist_plx_Pleiades.jpg
  • case1_Xray_source.jpg

  • Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image.

IPHAS and 2MASS color-color diagrams for matched point sources (case 4) selected in a box 1 degree wide and centred at ra=38.78 and deg=61.43

Changed:
<
<
>
>
Added:
>
>
    • Use case 5: The field of streams
 
META FILEATTACHMENT attachment="vospec.jpg" attr="" comment="Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec" date="1238599014" name="vospec.jpg" path="vospec.jpg" size="35840" stream="vospec.jpg" tmpFilename="/var/tmp/CGItemp8489" user="AngelaBragaglia" version="1"
META FILEATTACHMENT attachment="tuvikene_streams.png" attr="" comment="Use Case 5: The Field of Streams" date="1238600244" name="tuvikene_streams.png" path="tuvikene_streams.png" size="130281" stream="tuvikene_streams.png" tmpFilename="/var/tmp/CGItemp13144" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="IMF_case.jpg" attr="" comment="Comparison of an observed SED with a theoretical model (Use Case 2)" date="1238600342" name="IMF_case.jpg" path="IMF_case.jpg" size="119348" stream="IMF_case.jpg" tmpFilename="/var/tmp/CGItemp13617" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="ana.jpg" attr="" comment="Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image." date="1238600640" name="ana.jpg" path="ana.jpg" size="204032" stream="ana.jpg" tmpFilename="/var/tmp/CGItemp10897" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin.jpg" attr="" comment="usercase1_a" date="1238600827" name="Aladin.jpg" path="Aladin.jpg" size="50624" stream="Aladin.jpg" tmpFilename="/var/tmp/CGItemp19521" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="histogram.jpg" attr="" comment="usercase1_b" date="1238600859" name="histogram.jpg" path="histogram.jpg" size="23756" stream="histogram.jpg" tmpFilename="/var/tmp/CGItemp19669" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="color_color2.jpg" attr="" comment="usercase1_c" date="1238600881" name="color_color2.jpg" path="color_color2.jpg" size="49936" stream="color_color2.jpg" tmpFilename="/var/tmp/CGItemp19704" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin_after.jpg" attr="" comment="usercase1_d" date="1238600911" name="Aladin_after.jpg" path="Aladin_after.jpg" size="68656" stream="Aladin_after.jpg" tmpFilename="/var/tmp/CGItemp19721" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="VO_galaxy.png" attr="" comment="Galaxy and some foreground point sources." date="1238601001" name="VO_galaxy.png" path="VO_galaxy.png" size="683047" stream="VO_galaxy.png" tmpFilename="/var/tmp/CGItemp13959" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="im_all.jpg" attr="" comment="An SDSS RGB image of NGC2420. Overplotted are the hot star candidates." date="1238601083" name="im_all.jpg" path="im_all.jpg" size="19206" stream="im_all.jpg" tmpFilename="/var/tmp/CGItemp4593" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="topcat_aladin.jpg" attr="" comment="Collaboration between TOPCAT and Aladin" date="1238601577" name="topcat_aladin.jpg" path="topcat_aladin.jpg" size="395760" stream="topcat_aladin.jpg" tmpFilename="/var/tmp/CGItemp7499" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_Xray_source.jpg" attr="" comment="The Xray sources in the field correspond to rhe bright stars." date="1238602079" name="case1_Xray_source.jpg" path="case1_Xray_source.jpg" size="26188" stream="case1_Xray_source.jpg" tmpFilename="/var/tmp/CGItemp13621" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades" attr="h" comment="Histogram of the paralax. Blue are the bright stars." date="1238602249" name="case1_hist_plx_Pleiades" path="case1_hist_plx_Pleiades" size="23089" stream="case1_hist_plx_Pleiades" tmpFilename="/var/tmp/CGItemp13498" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Virgo2808.png" attr="" comment="Virgo : NGC2808 & search for dataset of high-res VLT spectra" date="1238602253" name="Virgo2808.png" path="Virgo2808.png" size="917789" stream="Virgo2808.png" tmpFilename="/var/tmp/CGItemp13232" user="AngelaBragaglia" version="1"
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades.jpg" attr="" comment="Histogram of the paralax. Blue are the bright stars." date="1238602468" name="case1_hist_plx_Pleiades.jpg" path="case1_hist_plx_Pleiades.jpg" size="23089" stream="case1_hist_plx_Pleiades.jpg" tmpFilename="/var/tmp/CGItemp13651" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Picture_5.png" attr="" comment="Halpha emitters in the IPHAS and 2MASS diagrams" date="1238658398" name="Picture_5.png" path="Picture 5.png" size="261604" stream="Picture 5.png" tmpFilename="/var/tmp/CGItemp9953" user="AidaSchool" version="1"

Revision 1002 Apr 2009 - Main.AidaSchool

 
META TOPICPARENT name="Gal1"

Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

Would be useful to delete a subset of table in Topcat.

Would be useful to have more than 4 tables to cross-match in TOPCAT

Would be useful to "remember" last scatter plot in TOPCAT, so we can use the same axes if we change from one table to a similar one

In Virgo: it would be useful to have different colours for the background and written parts (black on gray is not very readable).

In Virgo: it would be useful to get a list of the pointings/exposures shown in Stellarium; it would help to choose them

In Virgo: it would be useful to see also PI and program ID when an exposure is selected; or even the possibility of selecting by PI/ID if known.

-- AidaSchool - 31 Mar 2009

  • Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec:
    vospec.jpg
  • Comparison of an observed SED with a theoretical model (Use Case 2)

  • An SDSS RGB image of NGC2420. Overplotted are the hot star candidates.:
    im_all.jpg
  • An example for the collaboration betweenTopcat and Aladin
  • topcat_aladin.jpg
  • case1_hist_plx_Pleiades.jpg
  • case1_Xray_source.jpg

  • Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image.

IPHAS and 2MASS color-color diagrams for matched point sources (case 4) selected in a box 1 degree wide and centred at ra=38.78 and deg=61.43

META FILEATTACHMENT attachment="vospec.jpg" attr="" comment="Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec" date="1238599014" name="vospec.jpg" path="vospec.jpg" size="35840" stream="vospec.jpg" tmpFilename="/var/tmp/CGItemp8489" user="AngelaBragaglia" version="1"
META FILEATTACHMENT attachment="tuvikene_streams.png" attr="" comment="Use Case 5: The Field of Streams" date="1238600244" name="tuvikene_streams.png" path="tuvikene_streams.png" size="130281" stream="tuvikene_streams.png" tmpFilename="/var/tmp/CGItemp13144" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="IMF_case.jpg" attr="" comment="Comparison of an observed SED with a theoretical model (Use Case 2)" date="1238600342" name="IMF_case.jpg" path="IMF_case.jpg" size="119348" stream="IMF_case.jpg" tmpFilename="/var/tmp/CGItemp13617" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="ana.jpg" attr="" comment="Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image." date="1238600640" name="ana.jpg" path="ana.jpg" size="204032" stream="ana.jpg" tmpFilename="/var/tmp/CGItemp10897" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin.jpg" attr="" comment="usercase1_a" date="1238600827" name="Aladin.jpg" path="Aladin.jpg" size="50624" stream="Aladin.jpg" tmpFilename="/var/tmp/CGItemp19521" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="histogram.jpg" attr="" comment="usercase1_b" date="1238600859" name="histogram.jpg" path="histogram.jpg" size="23756" stream="histogram.jpg" tmpFilename="/var/tmp/CGItemp19669" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="color_color2.jpg" attr="" comment="usercase1_c" date="1238600881" name="color_color2.jpg" path="color_color2.jpg" size="49936" stream="color_color2.jpg" tmpFilename="/var/tmp/CGItemp19704" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin_after.jpg" attr="" comment="usercase1_d" date="1238600911" name="Aladin_after.jpg" path="Aladin_after.jpg" size="68656" stream="Aladin_after.jpg" tmpFilename="/var/tmp/CGItemp19721" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="VO_galaxy.png" attr="" comment="Galaxy and some foreground point sources." date="1238601001" name="VO_galaxy.png" path="VO_galaxy.png" size="683047" stream="VO_galaxy.png" tmpFilename="/var/tmp/CGItemp13959" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="im_all.jpg" attr="" comment="An SDSS RGB image of NGC2420. Overplotted are the hot star candidates." date="1238601083" name="im_all.jpg" path="im_all.jpg" size="19206" stream="im_all.jpg" tmpFilename="/var/tmp/CGItemp4593" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="topcat_aladin.jpg" attr="" comment="Collaboration between TOPCAT and Aladin" date="1238601577" name="topcat_aladin.jpg" path="topcat_aladin.jpg" size="395760" stream="topcat_aladin.jpg" tmpFilename="/var/tmp/CGItemp7499" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_Xray_source.jpg" attr="" comment="The Xray sources in the field correspond to rhe bright stars." date="1238602079" name="case1_Xray_source.jpg" path="case1_Xray_source.jpg" size="26188" stream="case1_Xray_source.jpg" tmpFilename="/var/tmp/CGItemp13621" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades" attr="h" comment="Histogram of the paralax. Blue are the bright stars." date="1238602249" name="case1_hist_plx_Pleiades" path="case1_hist_plx_Pleiades" size="23089" stream="case1_hist_plx_Pleiades" tmpFilename="/var/tmp/CGItemp13498" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Virgo2808.png" attr="" comment="Virgo : NGC2808 & search for dataset of high-res VLT spectra" date="1238602253" name="Virgo2808.png" path="Virgo2808.png" size="917789" stream="Virgo2808.png" tmpFilename="/var/tmp/CGItemp13232" user="AngelaBragaglia" version="1"
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades.jpg" attr="" comment="Histogram of the paralax. Blue are the bright stars." date="1238602468" name="case1_hist_plx_Pleiades.jpg" path="case1_hist_plx_Pleiades.jpg" size="23089" stream="case1_hist_plx_Pleiades.jpg" tmpFilename="/var/tmp/CGItemp13651" user="AidaSchool" version="1"
Added:
>
>
META FILEATTACHMENT attachment="Picture_5.png" attr="" comment="Halpha emitters in the IPHAS and 2MASS diagrams" date="1238658398" name="Picture_5.png" path="Picture 5.png" size="261604" stream="Picture 5.png" tmpFilename="/var/tmp/CGItemp9953" user="AidaSchool" version="1"
 

Revision 902 Apr 2009 - Main.AidaSchool

 
META TOPICPARENT name="Gal1"

Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

Would be useful to delete a subset of table in Topcat.

Would be useful to have more than 4 tables to cross-match in TOPCAT

Would be useful to "remember" last scatter plot in TOPCAT, so we can use the same axes if we change from one table to a similar one

In Virgo: it would be useful to have different colours for the background and written parts (black on gray is not very readable).

In Virgo: it would be useful to get a list of the pointings/exposures shown in Stellarium; it would help to choose them

In Virgo: it would be useful to see also PI and program ID when an exposure is selected; or even the possibility of selecting by PI/ID if known.

-- AidaSchool - 31 Mar 2009

  • Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec:
    vospec.jpg
  • Comparison of an observed SED with a theoretical model (Use Case 2)

  • An SDSS RGB image of NGC2420. Overplotted are the hot star candidates.:
    im_all.jpg
  • An example for the collaboration betweenTopcat and Aladin
  • topcat_aladin.jpg
  • case1_hist_plx_Pleiades.jpg
Added:
>
>
  • case1_Xray_source.jpg
 

  • Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image.
Changed:
<
<
IPHAS and 2MASS color-color diagrams for matched point sources (case 4) selected in a box 1 degree wide and centred at ra=38.78 and deg=61.43
>
>
IPHAS and 2MASS color-color diagrams for matched point sources (case 4) selected in a box 1 degree wide and centred at ra=38.78 and deg=61.43
 

META FILEATTACHMENT attachment="vospec.jpg" attr="" comment="Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec" date="1238599014" name="vospec.jpg" path="vospec.jpg" size="35840" stream="vospec.jpg" tmpFilename="/var/tmp/CGItemp8489" user="AngelaBragaglia" version="1"
META FILEATTACHMENT attachment="tuvikene_streams.png" attr="" comment="Use Case 5: The Field of Streams" date="1238600244" name="tuvikene_streams.png" path="tuvikene_streams.png" size="130281" stream="tuvikene_streams.png" tmpFilename="/var/tmp/CGItemp13144" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="IMF_case.jpg" attr="" comment="Comparison of an observed SED with a theoretical model (Use Case 2)" date="1238600342" name="IMF_case.jpg" path="IMF_case.jpg" size="119348" stream="IMF_case.jpg" tmpFilename="/var/tmp/CGItemp13617" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="ana.jpg" attr="" comment="Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image." date="1238600640" name="ana.jpg" path="ana.jpg" size="204032" stream="ana.jpg" tmpFilename="/var/tmp/CGItemp10897" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin.jpg" attr="" comment="usercase1_a" date="1238600827" name="Aladin.jpg" path="Aladin.jpg" size="50624" stream="Aladin.jpg" tmpFilename="/var/tmp/CGItemp19521" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="histogram.jpg" attr="" comment="usercase1_b" date="1238600859" name="histogram.jpg" path="histogram.jpg" size="23756" stream="histogram.jpg" tmpFilename="/var/tmp/CGItemp19669" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="color_color2.jpg" attr="" comment="usercase1_c" date="1238600881" name="color_color2.jpg" path="color_color2.jpg" size="49936" stream="color_color2.jpg" tmpFilename="/var/tmp/CGItemp19704" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin_after.jpg" attr="" comment="usercase1_d" date="1238600911" name="Aladin_after.jpg" path="Aladin_after.jpg" size="68656" stream="Aladin_after.jpg" tmpFilename="/var/tmp/CGItemp19721" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="VO_galaxy.png" attr="" comment="Galaxy and some foreground point sources." date="1238601001" name="VO_galaxy.png" path="VO_galaxy.png" size="683047" stream="VO_galaxy.png" tmpFilename="/var/tmp/CGItemp13959" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="im_all.jpg" attr="" comment="An SDSS RGB image of NGC2420. Overplotted are the hot star candidates." date="1238601083" name="im_all.jpg" path="im_all.jpg" size="19206" stream="im_all.jpg" tmpFilename="/var/tmp/CGItemp4593" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="topcat_aladin.jpg" attr="" comment="Collaboration between TOPCAT and Aladin" date="1238601577" name="topcat_aladin.jpg" path="topcat_aladin.jpg" size="395760" stream="topcat_aladin.jpg" tmpFilename="/var/tmp/CGItemp7499" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_Xray_source.jpg" attr="" comment="The Xray sources in the field correspond to rhe bright stars." date="1238602079" name="case1_Xray_source.jpg" path="case1_Xray_source.jpg" size="26188" stream="case1_Xray_source.jpg" tmpFilename="/var/tmp/CGItemp13621" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades" attr="h" comment="Histogram of the paralax. Blue are the bright stars." date="1238602249" name="case1_hist_plx_Pleiades" path="case1_hist_plx_Pleiades" size="23089" stream="case1_hist_plx_Pleiades" tmpFilename="/var/tmp/CGItemp13498" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Virgo2808.png" attr="" comment="Virgo : NGC2808 & search for dataset of high-res VLT spectra" date="1238602253" name="Virgo2808.png" path="Virgo2808.png" size="917789" stream="Virgo2808.png" tmpFilename="/var/tmp/CGItemp13232" user="AngelaBragaglia" version="1"
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades.jpg" attr="" comment="Histogram of the paralax. Blue are the bright stars." date="1238602468" name="case1_hist_plx_Pleiades.jpg" path="case1_hist_plx_Pleiades.jpg" size="23089" stream="case1_hist_plx_Pleiades.jpg" tmpFilename="/var/tmp/CGItemp13651" user="AidaSchool" version="1"

Revision 801 Apr 2009 - Main.AidaSchool

 
META TOPICPARENT name="Gal1"

Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

Would be useful to delete a subset of table in Topcat.

Would be useful to have more than 4 tables to cross-match in TOPCAT

Would be useful to "remember" last scatter plot in TOPCAT, so we can use the same axes if we change from one table to a similar one

In Virgo: it would be useful to have different colours for the background and written parts (black on gray is not very readable).

In Virgo: it would be useful to get a list of the pointings/exposures shown in Stellarium; it would help to choose them

In Virgo: it would be useful to see also PI and program ID when an exposure is selected; or even the possibility of selecting by PI/ID if known.

-- AidaSchool - 31 Mar 2009

  • Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec:
    vospec.jpg
  • Comparison of an observed SED with a theoretical model (Use Case 2)

  • An SDSS RGB image of NGC2420. Overplotted are the hot star candidates.:
    im_all.jpg
  • An example for the collaboration betweenTopcat and Aladin
Changed:
<
<
topcat_aladin.jpg
>
>
  • topcat_aladin.jpg
Added:
>
>
  • case1_hist_plx_Pleiades.jpg
 
Changed:
<
<
  • Virgo : NGC2808 & search for dataset of high-res VLT spectra:
>
>
Deleted:
<
<
Virgo2808.png
 
Added:
>
>
  • Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image.

IPHAS and 2MASS color-color diagrams for matched point sources (case 4) selected in a box 1 degree wide and centred at ra=38.78 and deg=61.43

 
META FILEATTACHMENT attachment="vospec.jpg" attr="" comment="Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec" date="1238599014" name="vospec.jpg" path="vospec.jpg" size="35840" stream="vospec.jpg" tmpFilename="/var/tmp/CGItemp8489" user="AngelaBragaglia" version="1"
META FILEATTACHMENT attachment="tuvikene_streams.png" attr="" comment="Use Case 5: The Field of Streams" date="1238600244" name="tuvikene_streams.png" path="tuvikene_streams.png" size="130281" stream="tuvikene_streams.png" tmpFilename="/var/tmp/CGItemp13144" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="IMF_case.jpg" attr="" comment="Comparison of an observed SED with a theoretical model (Use Case 2)" date="1238600342" name="IMF_case.jpg" path="IMF_case.jpg" size="119348" stream="IMF_case.jpg" tmpFilename="/var/tmp/CGItemp13617" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="ana.jpg" attr="" comment="Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image." date="1238600640" name="ana.jpg" path="ana.jpg" size="204032" stream="ana.jpg" tmpFilename="/var/tmp/CGItemp10897" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin.jpg" attr="" comment="usercase1_a" date="1238600827" name="Aladin.jpg" path="Aladin.jpg" size="50624" stream="Aladin.jpg" tmpFilename="/var/tmp/CGItemp19521" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="histogram.jpg" attr="" comment="usercase1_b" date="1238600859" name="histogram.jpg" path="histogram.jpg" size="23756" stream="histogram.jpg" tmpFilename="/var/tmp/CGItemp19669" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="color_color2.jpg" attr="" comment="usercase1_c" date="1238600881" name="color_color2.jpg" path="color_color2.jpg" size="49936" stream="color_color2.jpg" tmpFilename="/var/tmp/CGItemp19704" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin_after.jpg" attr="" comment="usercase1_d" date="1238600911" name="Aladin_after.jpg" path="Aladin_after.jpg" size="68656" stream="Aladin_after.jpg" tmpFilename="/var/tmp/CGItemp19721" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="VO_galaxy.png" attr="" comment="Galaxy and some foreground point sources." date="1238601001" name="VO_galaxy.png" path="VO_galaxy.png" size="683047" stream="VO_galaxy.png" tmpFilename="/var/tmp/CGItemp13959" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="im_all.jpg" attr="" comment="An SDSS RGB image of NGC2420. Overplotted are the hot star candidates." date="1238601083" name="im_all.jpg" path="im_all.jpg" size="19206" stream="im_all.jpg" tmpFilename="/var/tmp/CGItemp4593" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="topcat_aladin.jpg" attr="" comment="Collaboration between TOPCAT and Aladin" date="1238601577" name="topcat_aladin.jpg" path="topcat_aladin.jpg" size="395760" stream="topcat_aladin.jpg" tmpFilename="/var/tmp/CGItemp7499" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_Xray_source.jpg" attr="" comment="The Xray sources in the field correspond to rhe bright stars." date="1238602079" name="case1_Xray_source.jpg" path="case1_Xray_source.jpg" size="26188" stream="case1_Xray_source.jpg" tmpFilename="/var/tmp/CGItemp13621" user="AidaSchool" version="1"
Changed:
<
<
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades" attr="" comment="Histogram of the paralax. Blue are the bright stars." date="1238602249" name="case1_hist_plx_Pleiades" path="case1_hist_plx_Pleiades" size="23089" stream="case1_hist_plx_Pleiades" tmpFilename="/var/tmp/CGItemp13498" user="AidaSchool" version="1"
>
>
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades" attr="h" comment="Histogram of the paralax. Blue are the bright stars." date="1238602249" name="case1_hist_plx_Pleiades" path="case1_hist_plx_Pleiades" size="23089" stream="case1_hist_plx_Pleiades" tmpFilename="/var/tmp/CGItemp13498" user="AidaSchool" version="1"
 
META FILEATTACHMENT attachment="Virgo2808.png" attr="" comment="Virgo : NGC2808 & search for dataset of high-res VLT spectra" date="1238602253" name="Virgo2808.png" path="Virgo2808.png" size="917789" stream="Virgo2808.png" tmpFilename="/var/tmp/CGItemp13232" user="AngelaBragaglia" version="1"
Added:
>
>
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades.jpg" attr="" comment="Histogram of the paralax. Blue are the bright stars." date="1238602468" name="case1_hist_plx_Pleiades.jpg" path="case1_hist_plx_Pleiades.jpg" size="23089" stream="case1_hist_plx_Pleiades.jpg" tmpFilename="/var/tmp/CGItemp13651" user="AidaSchool" version="1"
 

Revision 701 Apr 2009 - Main.AngelaBragaglia

 
META TOPICPARENT name="Gal1"

Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

Would be useful to delete a subset of table in Topcat.

Would be useful to have more than 4 tables to cross-match in TOPCAT

Would be useful to "remember" last scatter plot in TOPCAT, so we can use the same axes if we change from one table to a similar one

In Virgo: it would be useful to have different colours for the background and written parts (black on gray is not very readable).

In Virgo: it would be useful to get a list of the pointings/exposures shown in Stellarium; it would help to choose them

In Virgo: it would be useful to see also PI and program ID when an exposure is selected; or even the possibility of selecting by PI/ID if known.

-- AidaSchool - 31 Mar 2009

  • Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec:
    vospec.jpg
  • Comparison of an observed SED with a theoretical model (Use Case 2)

  • An SDSS RGB image of NGC2420. Overplotted are the hot star candidates.:
    im_all.jpg
  • An example for the collaboration betweenTopcat and Aladin
topcat_aladin.jpg
Added:
>
>
  • Virgo : NGC2808 & search for dataset of high-res VLT spectra:
    Virgo2808.png
 
META FILEATTACHMENT attachment="vospec.jpg" attr="" comment="Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec" date="1238599014" name="vospec.jpg" path="vospec.jpg" size="35840" stream="vospec.jpg" tmpFilename="/var/tmp/CGItemp8489" user="AngelaBragaglia" version="1"
META FILEATTACHMENT attachment="tuvikene_streams.png" attr="" comment="Use Case 5: The Field of Streams" date="1238600244" name="tuvikene_streams.png" path="tuvikene_streams.png" size="130281" stream="tuvikene_streams.png" tmpFilename="/var/tmp/CGItemp13144" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="IMF_case.jpg" attr="" comment="Comparison of an observed SED with a theoretical model (Use Case 2)" date="1238600342" name="IMF_case.jpg" path="IMF_case.jpg" size="119348" stream="IMF_case.jpg" tmpFilename="/var/tmp/CGItemp13617" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="ana.jpg" attr="" comment="Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image." date="1238600640" name="ana.jpg" path="ana.jpg" size="204032" stream="ana.jpg" tmpFilename="/var/tmp/CGItemp10897" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin.jpg" attr="" comment="usercase1_a" date="1238600827" name="Aladin.jpg" path="Aladin.jpg" size="50624" stream="Aladin.jpg" tmpFilename="/var/tmp/CGItemp19521" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="histogram.jpg" attr="" comment="usercase1_b" date="1238600859" name="histogram.jpg" path="histogram.jpg" size="23756" stream="histogram.jpg" tmpFilename="/var/tmp/CGItemp19669" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="color_color2.jpg" attr="" comment="usercase1_c" date="1238600881" name="color_color2.jpg" path="color_color2.jpg" size="49936" stream="color_color2.jpg" tmpFilename="/var/tmp/CGItemp19704" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin_after.jpg" attr="" comment="usercase1_d" date="1238600911" name="Aladin_after.jpg" path="Aladin_after.jpg" size="68656" stream="Aladin_after.jpg" tmpFilename="/var/tmp/CGItemp19721" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="VO_galaxy.png" attr="" comment="Galaxy and some foreground point sources." date="1238601001" name="VO_galaxy.png" path="VO_galaxy.png" size="683047" stream="VO_galaxy.png" tmpFilename="/var/tmp/CGItemp13959" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="im_all.jpg" attr="" comment="An SDSS RGB image of NGC2420. Overplotted are the hot star candidates." date="1238601083" name="im_all.jpg" path="im_all.jpg" size="19206" stream="im_all.jpg" tmpFilename="/var/tmp/CGItemp4593" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="topcat_aladin.jpg" attr="" comment="Collaboration between TOPCAT and Aladin" date="1238601577" name="topcat_aladin.jpg" path="topcat_aladin.jpg" size="395760" stream="topcat_aladin.jpg" tmpFilename="/var/tmp/CGItemp7499" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_Xray_source.jpg" attr="" comment="The Xray sources in the field correspond to rhe bright stars." date="1238602079" name="case1_Xray_source.jpg" path="case1_Xray_source.jpg" size="26188" stream="case1_Xray_source.jpg" tmpFilename="/var/tmp/CGItemp13621" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades" attr="" comment="Histogram of the paralax. Blue are the bright stars." date="1238602249" name="case1_hist_plx_Pleiades" path="case1_hist_plx_Pleiades" size="23089" stream="case1_hist_plx_Pleiades" tmpFilename="/var/tmp/CGItemp13498" user="AidaSchool" version="1"
Added:
>
>
META FILEATTACHMENT attachment="Virgo2808.png" attr="" comment="Virgo : NGC2808 & search for dataset of high-res VLT spectra" date="1238602253" name="Virgo2808.png" path="Virgo2808.png" size="917789" stream="Virgo2808.png" tmpFilename="/var/tmp/CGItemp13232" user="AngelaBragaglia" version="1"
 

Revision 601 Apr 2009 - Main.AidaSchool

 
META TOPICPARENT name="Gal1"

Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

Would be useful to delete a subset of table in Topcat.

Would be useful to have more than 4 tables to cross-match in TOPCAT

Would be useful to "remember" last scatter plot in TOPCAT, so we can use the same axes if we change from one table to a similar one

In Virgo: it would be useful to have different colours for the background and written parts (black on gray is not very readable).

In Virgo: it would be useful to get a list of the pointings/exposures shown in Stellarium; it would help to choose them

In Virgo: it would be useful to see also PI and program ID when an exposure is selected; or even the possibility of selecting by PI/ID if known.

-- AidaSchool - 31 Mar 2009

  • Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec:
    vospec.jpg
Added:
>
>
  • Comparison of an observed SED with a theoretical model (Use Case 2)
 
Added:
>
>

  • An SDSS RGB image of NGC2420. Overplotted are the hot star candidates.:
    im_all.jpg
  • An example for the collaboration betweenTopcat and Aladin
topcat_aladin.jpg
 
META FILEATTACHMENT attachment="vospec.jpg" attr="" comment="Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec" date="1238599014" name="vospec.jpg" path="vospec.jpg" size="35840" stream="vospec.jpg" tmpFilename="/var/tmp/CGItemp8489" user="AngelaBragaglia" version="1"
Added:
>
>
META FILEATTACHMENT attachment="tuvikene_streams.png" attr="" comment="Use Case 5: The Field of Streams" date="1238600244" name="tuvikene_streams.png" path="tuvikene_streams.png" size="130281" stream="tuvikene_streams.png" tmpFilename="/var/tmp/CGItemp13144" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="IMF_case.jpg" attr="" comment="Comparison of an observed SED with a theoretical model (Use Case 2)" date="1238600342" name="IMF_case.jpg" path="IMF_case.jpg" size="119348" stream="IMF_case.jpg" tmpFilename="/var/tmp/CGItemp13617" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="ana.jpg" attr="" comment="Example of setting the WCS to an old (1936) Pleiades plate by the use of Aladin, USNO-A2 catalogue and POSS. Then running S-ex on the POSS2UKSTU _B image." date="1238600640" name="ana.jpg" path="ana.jpg" size="204032" stream="ana.jpg" tmpFilename="/var/tmp/CGItemp10897" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin.jpg" attr="" comment="usercase1_a" date="1238600827" name="Aladin.jpg" path="Aladin.jpg" size="50624" stream="Aladin.jpg" tmpFilename="/var/tmp/CGItemp19521" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="histogram.jpg" attr="" comment="usercase1_b" date="1238600859" name="histogram.jpg" path="histogram.jpg" size="23756" stream="histogram.jpg" tmpFilename="/var/tmp/CGItemp19669" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="color_color2.jpg" attr="" comment="usercase1_c" date="1238600881" name="color_color2.jpg" path="color_color2.jpg" size="49936" stream="color_color2.jpg" tmpFilename="/var/tmp/CGItemp19704" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="Aladin_after.jpg" attr="" comment="usercase1_d" date="1238600911" name="Aladin_after.jpg" path="Aladin_after.jpg" size="68656" stream="Aladin_after.jpg" tmpFilename="/var/tmp/CGItemp19721" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="VO_galaxy.png" attr="" comment="Galaxy and some foreground point sources." date="1238601001" name="VO_galaxy.png" path="VO_galaxy.png" size="683047" stream="VO_galaxy.png" tmpFilename="/var/tmp/CGItemp13959" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="im_all.jpg" attr="" comment="An SDSS RGB image of NGC2420. Overplotted are the hot star candidates." date="1238601083" name="im_all.jpg" path="im_all.jpg" size="19206" stream="im_all.jpg" tmpFilename="/var/tmp/CGItemp4593" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="topcat_aladin.jpg" attr="" comment="Collaboration between TOPCAT and Aladin" date="1238601577" name="topcat_aladin.jpg" path="topcat_aladin.jpg" size="395760" stream="topcat_aladin.jpg" tmpFilename="/var/tmp/CGItemp7499" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_Xray_source.jpg" attr="" comment="The Xray sources in the field correspond to rhe bright stars." date="1238602079" name="case1_Xray_source.jpg" path="case1_Xray_source.jpg" size="26188" stream="case1_Xray_source.jpg" tmpFilename="/var/tmp/CGItemp13621" user="AidaSchool" version="1"
META FILEATTACHMENT attachment="case1_hist_plx_Pleiades" attr="" comment="Histogram of the paralax. Blue are the bright stars." date="1238602249" name="case1_hist_plx_Pleiades" path="case1_hist_plx_Pleiades" size="23089" stream="case1_hist_plx_Pleiades" tmpFilename="/var/tmp/CGItemp13498" user="AidaSchool" version="1"
 

Revision 501 Apr 2009 - Main.AngelaBragaglia

 
META TOPICPARENT name="Gal1"

Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

Would be useful to delete a subset of table in Topcat.

Changed:
<
<
Would be useful to have more than 4 tables to cross-match in TOPCAT
>
>
Would be useful to have more than 4 tables to cross-match in TOPCAT
 
Added:
>
>
Would be useful to "remember" last scatter plot in TOPCAT, so we can use the same axes if we change from one table to a similar one
 In Virgo: it would be useful to have different colours for the background and written parts (black on gray is not very readable).

In Virgo: it would be useful to get a list of the pointings/exposures shown in Stellarium; it would help to choose them

In Virgo: it would be useful to see also PI and program ID when an exposure is selected; or even the possibility of selecting by PI/ID if known.

-- AidaSchool - 31 Mar 2009

Added:
>
>
  • Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec:
    vospec.jpg

META FILEATTACHMENT attachment="vospec.jpg" attr="" comment="Example of a UVES spectrum (ESO-highly processed data) retrieved by VOSpec" date="1238599014" name="vospec.jpg" path="vospec.jpg" size="35840" stream="vospec.jpg" tmpFilename="/var/tmp/CGItemp8489" user="AngelaBragaglia" version="1"

Revision 401 Apr 2009 - Main.AngelaBragaglia

 
META TOPICPARENT name="Gal1"

Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

Would be useful to delete a subset of table in Topcat.

Would be useful to have more than 4 tables to cross-match in TOPCAT

Added:
>
>
In Virgo: it would be useful to have different colours for the background and written parts (black on gray is not very readable).

In Virgo: it would be useful to get a list of the pointings/exposures shown in Stellarium; it would help to choose them

In Virgo: it would be useful to see also PI and program ID when an exposure is selected; or even the possibility of selecting by PI/ID if known.

  -- AidaSchool - 31 Mar 2009

Revision 301 Apr 2009 - Main.AngelaBragaglia

 
META TOPICPARENT name="Gal1"

Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

Changed:
<
<
Would be useful to delete a subset of table in Topcat.
>
>
Would be useful to delete a subset of table in Topcat.
Added:
>
>
Would be useful to have more than 4 tables to cross-match in TOPCAT
  -- AidaSchool - 31 Mar 2009

Revision 231 Mar 2009 - Main.AidaSchool

 
META TOPICPARENT name="Gal1"

Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

Changed:
<
<
-- AidaSchool - 31 Mar 2009
>
>
Would be useful to delete a subset of table in Topcat.
 
Added:
>
>
-- AidaSchool - 31 Mar 2009

Revision 131 Mar 2009 - Main.AidaSchool

 
META TOPICPARENT name="Gal1"

Gal One - Notes and Comments

Comments on Software

Would be useful to have an UNDO function on say topcat, aladin

-- AidaSchool - 31 Mar 2009

 
This site is powered by the TWiki collaboration platformCopyright © by the contributing authors. All material on this collaboration platform is the property of the contributing authors.
Ideas, requests, problems regarding TWiki? Send feedback